Distributions of ⟨M^*⟩, ⟨SFR⟩, ⟨sSFR⟩, ⟨θ⟩, ⟨cos(4θ)⟩, fraction of quenched galaxies (f_Q), fraction of ordered galaxies (f_Ord), fraction of parallel galaxies (f_∥), and fraction of perpendicular galaxies (f_⊥) as a function of the distances from the features of the cosmic web d_fil (red line in every panel), d_CP (blue line in every panel), and d_skel (orange line in every panel) and split between high- and low-mass galaxies. In the case of d_CP and d_skel, only galaxies outside of filaments (d_fil ≥ 1 Mpc) and inside filaments (d_fil ≤ 1 Mpc) have been considered, respectively. Error bars on the distributions have been computed through bootstrap resampling. The dashed (dotted) black line in every panel is the average of the considered quantity in the full simulation box considering only high-mass (low-mass) galaxies. In the top and middle panel of the central column, the grey line is and , computed given equations (3) and (4) for the total subhalo sample. In each panel, solid lines refer to high-mass galaxies and dashed lines to low-mass galaxies. In the case of mass, sSFR, and f_Q, the panel has been split into two to take into account the very different ranges on the y-axis occupied by the distributions. Only high-spin parameter subhaloes are used to derive the distributions selected using the Bullock parameter computed using only particles within the R₂₀₀ of subhaloes. In every panel the first distance bin considered extends all the way to zero for all distances, but it is cut because the x-axis is in logarithmic scale. In the f_∥ and f_⊥ cases, the y-axes of the plots cover very different ranges.